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Curriculum Vitae for MERCEDES T. RICHARDS
Curriculum Vitae for MERCEDES T. RICHARDS Work Address: Department of Astronomy & Astrophysics, Penn State University, 525 Davey Lab, University Park, PA 16802-6305 Telephone: (814) 865-0150 (office); (814) 863-3399 (fax) E-mail address: [email protected] Web address: http://www.astro.psu.edu/~mrichards Education Ph.D., 1986, Astronomy, University of Toronto M.Sc., 1979, Astronomy, York University B.Sc., 1977, Physics, University of the West Indies Graduate Awards: University of the West Indies Graduate Scholarship, 1977-1979; York University Scholarship, 1977-1979; University of Toronto Doctoral Fellowship, 1979-1981; Frank Hogg Fellowship, 1981-1982; C. A. Chant Fellowship, 1982-1983; Carl Reinhardt Fellowship, 1981-1986. Academic Positions 2003 – : Assistant Head, Department of Astronomy & Astrophysics, Penn State University 2002 – : Professor, Department of Astronomy & Astrophysics, Penn State University 2000 – 2001: Visiting Scientist, Institute for Advanced Study, Princeton 1999 – 2002: Professor, Department of Astronomy, University of Virginia 1993 – 1999: Associate Professor, Department of Astronomy, University of Virginia 1987 – 1993: Assistant Professor, Department of Astronomy, University of Virginia 1986 – 1987: Visiting Scholar, Dept. of Physics & Astronomy, U. North Carolina, Chapel Hill 1979 – 1985: Teaching Assistant, Department of Astronomy, University of Toronto, Canada 1977 – 1979: Research/Teaching Assistant, Centre for Research in Earth & Space Science, York University Academic Service Positions 2007 – 2010: -
Evans.2013.HD189733.Albedo.Pdf
ORE Open Research Exeter TITLE The Deep Blue Color of HD 189733b: Albedo Measurements with Hubble Space Telescope/Space Telescope Imaging Spectrograph at Visible Wavelengths AUTHORS Evans, T.M.; Pont, F.; Sing, David K.; et al. JOURNAL Astrophysical Journal DEPOSITED IN ORE 15 December 2014 This version available at http://hdl.handle.net/10871/16042 COPYRIGHT AND REUSE Open Research Exeter makes this work available in accordance with publisher policies. A NOTE ON VERSIONS The version presented here may differ from the published version. If citing, you are advised to consult the published version for pagination, volume/issue and date of publication The Astrophysical Journal Letters, 772:L16 (5pp), 2013 August 1 doi:10.1088/2041-8205/772/2/L16 C 2013. The American Astronomical Society. All rights reserved. Printed in the U.S.A. THE DEEP BLUE COLOR OF HD 189733b: ALBEDO MEASUREMENTS WITH HUBBLE SPACE TELESCOPE/SPACE TELESCOPE IMAGING SPECTROGRAPH AT VISIBLE WAVELENGTHS Thomas M. Evans1,Fred´ eric´ Pont2,DavidK.Sing2, Suzanne Aigrain1, Joanna K. Barstow1, Jean-Michel Desert´ 3,7, Neale Gibson4, Kevin Heng5, Heather A. Knutson3, and Alain Lecavelier des Etangs6 1 Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK; [email protected] 2 School of Physics, University of Exeter, EX4 4QL Exeter, UK 3 Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA 4 European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching, Germany 5 University of Bern, Center for Space and Habitability, Sidlerstrasse 5, CH-3012 Bern, Switzerland 6 Institut d’Astrophysique de Paris, UMR7095 CNRS, Universite Pierre et Marie Curie, 98 bis Boulevard Arago, F-75014 Paris, France Received 2013 May 31; accepted 2013 June 15; published 2013 July 11 ABSTRACT We present a secondary eclipse observation for the hot Jupiter HD 189733b across the wavelength range 290–570 nm made using the Space Telescope Imaging Spectrograph on the Hubble Space Telescope. -
Javier Peralta Calvillo Generated From: Editor CVN De FECYT Date of Document: 24/01/2021 V 1.4.3 4154B7e2be6a86b67f637261e4ad3d11
Javier Peralta Calvillo Generated from: Editor CVN de FECYT Date of document: 24/01/2021 v 1.4.3 4154b7e2be6a86b67f637261e4ad3d11 This electronic file (PDF) has embedded CVN technology (CVN-XML). The CVN technology of this file allows you to export and import curricular data from and to any compatible data base. List of adapted databases available at: http://cvn.fecyt.es/ 4154b7e2be6a86b67f637261e4ad3d11 General quality indicators of scientific research This section describes briefly the main quality indicators of scientific production (periods of research activity, experience in supervising doctoral theses, total citations, articles in journals of the first quartile, H index...). It also includes other important aspects or peculiarities. My name is Javier Peralta and I was born in Algeciras (1979, Spain). I graduated in Physics at the University of La Laguna (Spain) in 2003, specializing in the fields of Astrophysics and Applied Physics. In 2009, I got an European PhD degree in Physics at the University of the Basque Country (Spain) with the highest qualification ("Cum Laude") . My PhD research, supervised by Professors Agustín Sánchez-Lavega and Ricardo Hueso, focused on the atmospheric dynamics of the planet Venus using data from the space missions Galileo and Venus Express. As a result, 6 articles were published in international peer review journals (4 of them as first author) along with more than 80 citations which allowed to be awarded in 2012 with the “Extraordinary Prize of Doctorate” granted by the University of the Basque Country. After my PhD, I spent the last 10 years (2009-2019) working in different research institutions as postdoctoral researcher: 2 years at IAA/CSIC in Granada (Spain), 3 years at the Astronomical Observatory of Lisbon (CAAUL/OAL, Portugal) and 5 years at the Institute of Space and Astronautical Science of Japan (ISAS/JAXA), funded by JAXA's International Top Young Fellowship (ITYF). -
Winter 2015 Greetings in May the Royal Society Bestowed Fellowship on Professor Yvonne Elsworth For
Winter 2015 Greetings In May the Royal Society bestowed Fellowship on Professor Yvonne Elsworth for her, “pioneering work in establishing and maintaining an important scientific investigation into the internal structure of the Sun using helioseismic data from the autonomous Birmingham network of observatories complemented by extant data from modes of intermediate degree has permitted an unprecedented investigation into the inner core of the Sun where the nuclear reactions are taking place.” This is well-deserved recognition both for Yvonne and the entire helioseismology group. They are now applying the technique that they pioneered to understanding the structure of stars around which Birmingham, as part of the Kepler mission, is now discovering new planets. Professor Yvonne Elsworth FRS, presenting one of our Physics Role Model seminars. These occur once a term, and are a personal reflection of people’s career paths (this was the first academic career to be showcased); what they are doing; and advice for their younger selves. Please contact us if you would be interested in giving one – we aim to present the diversity of careers possible with a Physics degree. The School and Particle Physics group also celebrated the retirement of Dr John Wilson. John joined the University of Birmingham in 1973 as a Research Fellow, becoming a Lecturer in 1982. He contributed to the work of the group at CERN, particularly the UA1 and Opal experiments, the former being linked to the discovery of the W+/- and Z0 particles – mediators of the weak interaction. John was famed for his contribution to instrumentation and most latterly his spark chamber, which fantastically illustrated the tracks of cosmic rays to a whole generation of School students. -
Benefactors 2020
Contents 2 From the President 4 From the Development Director 6 Your Gifts 8 Graduate Scholars 12 Special Grants 18 Access and Outreach 22 Buildings 26 Why I Give 30 Financial Report 32 Roll of Benefactors Including Summary Financial Report, Sources and Use of Funds for the year 2018–19 Benefactors is now plastic free and can be recycled with your usual household paper recycling. The mailing bag is made of a compostable plastic-free material. 1 From the President St John’s continues to make progress on all fronts and I’m delighted to be able to share our news in this edition of Benefactors. This academic year we are celebrating the 40th anniversary will be independent evaluation of the effectiveness of since women were first admitted to St John’s. The this programme and we are hopeful that we have a great programme of events has been interesting and thought- model that can deliver a significant impact and that could provoking and has put a clear focus on issues of diversity, be rolled out more widely. equality and inclusion, not only in our day-to-day activities in College but also in our continuing efforts to attract the It was excellent to celebrate the opening of the new Study brightest and best to St John’s, irrespective of background. Centre last October and a wonderful opportunity to thank the donors who helped make the project happen. The College – and the University overall – are making We continue to invest substantially in the renovation significant progress on access. You may be aware of of College buildings with work in 2020 on St Giles the new Opportunity Oxford programme: students House, a redesign of the Lodge, and on the third and invited onto Opportunity Oxford are made the standard final phase of the Library project, including conservation offer for their course and then take part in a supportive improvements to the Old Library and Laudian Library bridging programme in the run-up to their first term. -
The Wonders of Star Formafion
The Wonders of Star Forma;on A tribute to Hans Zinnecker Edinburgh, Scotland 3-7 September, 2018 i John McIntyre Conference Centre Edinburgh UK 3rd - 7th September 2018 SOC Anthony Whitworth (Cardiff, UK, Co-Chair) Ken Rice (Edinburgh, UK, Co-Chair) Bo Reipurth (Hawaii, USA) Cathie Clarke (Cambridge, UK) Ian Bonnell (St Andrews, UK) Mark McCaughrean (ESA) Stephanie Walch (Cologne, Germany) Hal Yorke (USRA, USA) John Bally (Colorado, USA) Dimitris Stamatellos (UCLAN, UK) LOC Lyndsey Ballantyne Ken Rice ii Contents General Information 1 Information for Speakers . .1 Information for Posters . .1 WiFi Access . .1 Social Media . .1 Open forum: The Challenges Ahead . .2 Timetable . .3 Floorplan . .4 Getting Around Edinburgh . .5 Dining Options . .6 Excursions . .7 Useful Information . .7 Code of Conduct . .8 Talk Abstracts 9 Poster List & Abstracts 87 iii iv General Information Information for Speakers You are welcome to use your own laptops, but we will also be providing a Mac with OS X and a Windows machine for speakers to use. We can accomodate PDF, Keynote and Powerpoint. Please ensure you have uploaded and tested your talk on the computers prior to your session beginning, or have tested your own laptop/device. All contributed talks are 15 minutes plus 5 minutes for questions, while invited review talks are 30 minutes plus 10 minutes for questions. Session chairs will give appropriate warnings when you are approaching your time limit. To ensure the smooth running of each session, please keep to time. Thank you! Information for Posters Posters are allocated a numbered board based on the session to which they've been allocated. -
For Digital Simulation and Advanced Computation 2002 Annual Research Report
for Digital Simulation and Advanced Computation 2002 Annual Research Report 2002 Annual Research Report of the Supercomputing Institute for Digital Simulation and Advanced Computation Visit us on the Internet: www.msi.umn.edu Supercomputing Institute for Digital Simulation and Advanced Computation University of Minnesota 599 Walter 117 Pleasant Street SE Minneapolis, Minnesota 55455 ©2002 by the Regents of the University of Minnesota. All rights reserved. This report was prepared by Supercomputing Institute researchers and staff. Editor: Tracey Bartlett This information is available in alternative formats upon request by individuals with disabilities. Please send email to [email protected] or call (612) 625-1818. The University of Minnesota is committed to the policy that all persons shall have equal access to its programs, facilities, and employment without regard to race, color, creed, religion, national origin, sex, age, marital status, disability, public assistance status, veteran status, or sex- ual orientation. contains a minimum of 10% postconsumer waste Table of Contents Introduction Supercomputing Resources Overview....................................................................................................................................2 Supercomputers ........................................................................................................................3 Research Laboratories and Programs ......................................................................................5 Supercomputing Institute -
Detection and Characterization of Oscillating Red Giants: First Results from the TESS Satellite
The Astrophysical Journal Letters, 889:L34 (8pp), 2020 February 1 https://doi.org/10.3847/2041-8213/ab6443 © 2020. The American Astronomical Society. All rights reserved. Detection and Characterization of Oscillating Red Giants: First Results from the TESS Satellite Víctor Silva Aguirre1 , Dennis Stello1,2,3 , Amalie Stokholm1 , Jakob R. Mosumgaard1 , Warrick H. Ball1,4 , Sarbani Basu5 , Diego Bossini6 , Lisa Bugnet7,8 , Derek Buzasi9 , Tiago L. Campante6,10 , Lindsey Carboneau9 , William J. Chaplin1,4 , Enrico Corsaro11 , Guy R. Davies1,4 , Yvonne Elsworth1,4, Rafael A. García7,8 , Patrick Gaulme12,13 , Oliver J. Hall1,4 , Rasmus Handberg1 , Marc Hon2 , Thomas Kallinger14 , Liu Kang15 , Mikkel N. Lund1 , Savita Mathur16,17 , Alexey Mints18 , Benoit Mosser19 , Zeynep Çelik Orhan20 , Thaíse S. Rodrigues21 , Mathieu Vrard6,22, Mutlu Yıldız20 , Joel C. Zinn2,22,23 , Sibel Örtel20 , Paul G. Beck16,17,24 , Keaton J. Bell25,62 , Zhao Guo26 , Chen Jiang27 , James S. Kuszlewicz12 , Charles A. Kuehn28, Tanda Li1,3,4, Mia S. Lundkvist1, Marc Pinsonneault22 , Jamie Tayar29,63 , Margarida S. Cunha4,6 , Saskia Hekker1,12 , Daniel Huber29, Andrea Miglio1,4 , Mario J. P. F. G. Monteiro6,10 , Ditte Slumstrup1,30 , Mark L. Winther1, George Angelou31 , Othman Benomar32,33 , Attila Bódi34,35, Bruno L. De Moura36, Sébastien Deheuvels37, Aliz Derekas34,38,39 , Maria Pia Di Mauro40 , Marc-Antoine Dupret41, Antonio Jiménez16,17, Yveline Lebreton19,42 , Jaymie Matthews43 , Nicolas Nardetto44 , Jose D. do Nascimento, Jr.45,46 , Filipe Pereira6,10 , Luisa F. Rodríguez Díaz1 , Aldo M. Serenelli47,48, Emanuele Spitoni1 , Edita Stonkutė49, Juan Carlos Suárez50,51, Robert Szabó34,35, Vincent Van Eylen52 , Rita Ventura11 , Kuldeep Verma1 , Achim Weiss31 , Tao Wu53,54,55 , Thomas Barclay56,57 , Jørgen Christensen-Dalsgaard1 , Jon M. -
Suzanne Aigrain on Behalf of the Corot Exoplanet Science Team Why Space?
Suzanne Aigrain on behalf of the CoRoT exoplanet science team Why space? • Atmosphere limits precision photometry from the ground • Scintillation limit ~2 mmag • Representative transit depths for Sun-like star • Jupiter: 10 mmag • Neptune: 1.3 mmag • Earth: 0.1 mmag • Weather and daytime limit temporal coverage from the ground • Many sources of noise transit timescales removed • colour dependent differential extinction, seeing, etc... 27 December 2006 The satellite • PI: Annie Baglin, LESIA, Meudon • CNES PROTEUS bus • 27cm aperture telescope • Soyuz II-1b launcher from Baikonour • Polar orbit • 2.5 year minimum lifetime Payload 27cm telescope layout focal box Full images, windowing and target selection Focal planeSeismology detector (Vincent Lapeyrere) Exopplnat detector (Farid Karioty) • Sismo field • 5 windows / CCD • 5.7 < mV < 9.5 • 32s sampling (1s on request) • frame transfer mode • used for astrometry 2.8° • 10 bright stars • 10 background windows • 11600 faint stars • 400 background windows CoRoT_Booklet_talks_summer2007 2 seismo exo SCAO Pointing stability Barycenter X of the stellar image x-coord of stellar image barycenter Stability performances : x axis: rms 0.12 pixel y axis: rms 0.15 pixel ~ 0RMS.3 a stability:rc sec. 0.12 pixel in x 0.15 pixel in y ~0.3 arcsec Vibrations due to the entrance and exit form ecclipses vibrations due to Earth eclipse ingress and egress CoRoT_Booklet_talks_summer2007 3 Exo field 2.8° • Exo field • up to 6000 LCs / CCD • 11.5 < mV < 16 • 512s sampling (32s for 500 objects / CCD) • 3 colours for -
Bondi-Hoyle Accretion
A Review of Bondi–Hoyle–Lyttleton Accretion Richard Edgar a aStockholms observatorium, AlbaNova universitetscentrum, SE-106 91, Stockholm, Sweden Abstract If a point mass moves through a uniform gas cloud, at what rate does it accrete ma- terial? This is the question studied by Bondi, Hoyle and Lyttleton. This paper draws together the work performed in this area since the problem was first studied. Time has shown that, despite the simplifications made, Bondi, Hoyle and Lyttleton made quite accurate predictions for the accretion rate. Bondi–Hoyle–Lyttleton accretion has found application in many fields of astronomy, and these are also discussed. Key words: accretion PACS: 95.30.Lz, 97.10.Gz, 98.35.Mp, 98.62.Mw 1 Introduction arXiv:astro-ph/0406166v2 21 Jun 2004 In its purest form, Bondi–Hoyle–Lyttleton accretion concerns the supersonic motion of a point mass through a gas cloud. The cloud is assumed to be free of self-gravity, and to be uniform at infinity. Gravity focuses material behind the point mass, which can then accrete some of the gas. This problem has found applications in many areas of astronomy, and this paper is an attempt to address the lack of a general review of the subject. I start with a short summary of the original work of Bondi, Hoyle and Lyt- tleton, followed by a discussion of the numerical simulations performed. Some issues in Bondi–Hoyle–Lyttleton accretion are discussed, before a brief sum- mary of the fields in which the geometry has proved useful. Email address: [email protected] (Richard Edgar). -
A Thesis Entitled Knotted Numbers, Mnemonics, and Narratives: Khipu
A Thesis entitled Knotted Numbers, Mnemonics, and Narratives: Khipu Scholarship and the Search for the “Khipu Code” throughout the Twentieth and Twenty First Century by Veronica Lysaght Submitted to the Graduate Faculty as partial fulfillment of the requirements for the Master of Arts Degree in History ________________________________________ Charles Beatty-Medina, Committee Chair ________________________________________ Roberto Padilla, Committee Member ________________________________________ Kim Nielsen, Committee Member _______________________________________ Amanda Bryant-Friedrich, Dean College of Graduate Studies The University of Toledo July 2016 Copyright 2016, Veronica Lee Lysaght This document is copyrighted material. Under copyright law, no parts of this document may be reproduced without the expressed permission of the author. An Abstract of Knotted Numbers, Mnemonics, and Narratives: Khipu Scholarship and the Search for the “Khipu Code” throughout the Twentieth and Twenty First Century by Veronica Lysaght Submitted to the Graduate Faculty as partial fulfillment of the requirements for the Master of Arts Degree in History The University of Toledo July 2016 My thesis explores the works of European and North American khipu scholars (mainly anthropologists) from 1912 until 2010. I analyze how they incorporated aspects of their own culture and values into their interpretations of Inca khipus’ structure and functions. As Incas did not leave behind a written language or even clear non-written descriptions of their khipus, anthropologists interpreted khipus’ purposes with a limited base of Inca perspectives. Thus, every work of khipu literature that I study reflects both elements of Inca culture and the author’s own cultural perspectives as a twentieth or twenty-first century academic. I show how each work is indicative of modern cultural views on writing, as well as academic movements and broader social trends that were prominent during the author’s time. -
10. Scientific Programme 10.1
10. SCIENTIFIC PROGRAMME 10.1. OVERVIEW (a) Invited Discourses Plenary Hall B 18:00-19:30 ID1 “The Zoo of Galaxies” Karen Masters, University of Portsmouth, UK Monday, 20 August ID2 “Supernovae, the Accelerating Cosmos, and Dark Energy” Brian Schmidt, ANU, Australia Wednesday, 22 August ID3 “The Herschel View of Star Formation” Philippe André, CEA Saclay, France Wednesday, 29 August ID4 “Past, Present and Future of Chinese Astronomy” Cheng Fang, Nanjing University, China Nanjing Thursday, 30 August (b) Plenary Symposium Review Talks Plenary Hall B (B) 8:30-10:00 Or Rooms 309A+B (3) IAUS 288 Astrophysics from Antarctica John Storey (3) Mon. 20 IAUS 289 The Cosmic Distance Scale: Past, Present and Future Wendy Freedman (3) Mon. 27 IAUS 290 Probing General Relativity using Accreting Black Holes Andy Fabian (B) Wed. 22 IAUS 291 Pulsars are Cool – seriously Scott Ransom (3) Thu. 23 Magnetars: neutron stars with magnetic storms Nanda Rea (3) Thu. 23 Probing Gravitation with Pulsars Michael Kremer (3) Thu. 23 IAUS 292 From Gas to Stars over Cosmic Time Mordacai-Mark Mac Low (B) Tue. 21 IAUS 293 The Kepler Mission: NASA’s ExoEarth Census Natalie Batalha (3) Tue. 28 IAUS 294 The Origin and Evolution of Cosmic Magnetism Bryan Gaensler (B) Wed. 29 IAUS 295 Black Holes in Galaxies John Kormendy (B) Thu. 30 (c) Symposia - Week 1 IAUS 288 Astrophysics from Antartica IAUS 290 Accretion on all scales IAUS 291 Neutron Stars and Pulsars IAUS 292 Molecular gas, Dust, and Star Formation in Galaxies (d) Symposia –Week 2 IAUS 289 Advancing the Physics of Cosmic